Star · F9
WASP-108
WASP-108 is a main-sequence star of spectral type F9 in the constellation Centaurus, 835.7 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Centaurus |
|---|---|
| Distance | 835.7 light-years (256.2 pc) |
| Apparent magnitude | magnitude 11.28 |
| Absolute magnitude | magnitude 4.24 |
| Spectral type | F9 |
| Surface temperature | 6,780 K |
| Luminosity | 2.08 L☉ |
| Radius | 1.34 R☉ |
| Mass | 1.17 M☉ |
| Age | 4.6 billion years |
| Metallicity [Fe/H] | 0.15 |
| Right ascension (J2000) | 13h 03m 18.7s |
| Declination (J2000) | −49° 38′ 23″ |
| Space velocity (relative to the Sun) | 41.5 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 11.28. Visible from the whole Southern Hemisphere and north to latitude 40° N. South of latitude 40° S it never sets. It stands highest at midnight in April, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1190. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 15 million years.
The Sun seen from there
From a planet around WASP-108, the Sun would look like a star of magnitude 11.87, in the direction where our sky has the constellation Cassiopeia. It would be invisible to the naked eye.
Planets
- WASP-108 b 2.68-day orbit · 15.1 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.